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Simulations of Polarimetric Radar Signatures of a Supercell Storm Using a Two-Moment Bulk Microphysics Scheme

机译:基于两步体微物理方案的超级单体风暴极化雷达特征仿真

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A new general polarimetric radar simulator for nonhydrostatic numerical weather prediction (NWP) models has been developed based on rigorous scattering calculations using the T-matrix method for reflectivity differential reflectivity, specific differential phase, and copolar cross-correlation coefficient. A continuous melting process accounts for the entire spectrum of varying density and dielectric constants. This simulator is able to simulate polarimetric radar measurements at weather radar frequency bands and can take as input the prognostic variables of high-resolution NWP model simulations using one-, two-, and three-moment microphysics schemes. The simulator was applied at 10.7-cm wavelength to a model-simulated supercell storm using a double-moment (two moment) bulk microphysics scheme to examine its ability to simulate polarimetric signatures reported in observational studies. The simulated fields exhibited realistic polarimetric signatures that include Z_(DR) and K_(DR) columns, Z_(DR) arc, midlevel Z_(DR) and p_(hv) rings, hail signature and K_(DP) foot in terms of their general location, shape, and strength. The authors compared the simulation with one employing a single-moment (SM) microphysics scheme and found that certain signatures,such as Z arc midlevel ZDR, and p_(hv) rings, cannot be reproduced with the latter. It is believed to be primarily caused by the limitation of the SM scheme in simulating the shift of the particle size distribution toward larger/smaller diameters, independent of mixing ratio. These results suggest that two- or higher-moment microphvsics schemes should be used to adequately describe certain important microphysical processes. They also demonstrate the utility of a well-designed radar simulator for validating numerical models. In addition, the simulator can also serve as a training tool for forecasters to recognize polarimetric signatures that can be reproduced by advanced NWP models.
机译:基于严格的散射计算,使用T矩阵方法针对反射率差分反射率,特定差分相位和同极互相关系数,开发了一种用于非静水数值天气预报(NWP)模型的新型通用极化雷达模拟器。连续熔化过程说明了密度和介电常数变化的整个光谱。该模拟器能够模拟气象雷达频段上的极化雷达测量结果,并且可以使用一阶,二阶和三阶微物理方案将高分辨率NWP模型模拟的预测变量作为输入。使用双矩(两刻)本体微物理方案将模拟器以10.7厘米波长应用于模型模拟的超级单体风暴,以检查其模拟观测研究中报告的极化特征的能力。模拟场表现出逼真的极化特征,包括Z_(DR)和K_(DR)列,Z_(DR)弧,中层Z_(DR)和p_(hv)环,冰雹特征和K_(DP)足一般位置,形状和强度。作者将模拟与采用单矩(SM)微物理学方案的模拟进行了比较,发现某些签名(例如Z弧中级ZDR和p_(hv)环)无法与后者重现。认为这主要是由于SM方案在模拟粒度分布向较大/较小直径的偏移方面的局限性所致,而与混合比无关。这些结果表明,应使用两个或更高时刻的微囊方案来充分描述某些重要的微物理过程。他们还演示了精心设计的雷达模拟器在验证数值模型中的实用性。此外,模拟器还可以用作预报员的培训工具,以识别可以由高级NWP模型重现的极化特征。

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